To solve the origin of the hard XRB, a long standing puzzle in X-ray astronomy, was one of the primary scientific goals to be addressed with ASCA.
From deep surveys, they resolved 35% and 80% the soft XRB into discrete sources.
They detected total 107 sources, with a flux limit of [10.sup.-13] erg [cm.sup.-2][s.sup.-1] in the 2-10 band, resolving 20-26% of the 2-10 keV XRB. (40) An important result is that they found evidence for the solution of the "spectral paradox" by detecting a significant fraction of sources with hard spectra.
Soon after the launch, Chandra resolved >75% of the hard XRB above 2 keV into discrete sources.
It is seen that a large fraction (~80%) of the XRB below 10 keV is now clearly resolved into faint, individual sources, mostly AGNs.
Pure cultures of the xylem residing bacteria (XRB) thus obtained were maintained at -80[degrees]C, as glycerol stocks for long term, and 4[degrees]C for temporary storage.
ARDRA was performed to determine the genetic diversity of the XRB in the collection.
One hundred and sixty-seven XRB were screened for inhibition of the BW pathogen.
Production of Volatile and Diffusible Antagonistic Substances by XRB
The XRB issued in September Accounting Standards Framework: A Multi Standards Approach and two consultation papers, including Accounting Standards Framework for General Purpose Financial Reporting by For-Profit Entities.
Large for-profit entities without public accountability would likely apply full NZ IFRS with reduced disclosures according to plans favored by the XRB.